Auroral potential structures and current-voltage relationship: summary of recent results

P. Janhunen , A. Olsson
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引用次数: 4

Abstract

Discrete auroral arcs are caused by precipitating accelerated electrons, and there is a lot of observational evidence for the associated potential structure being U-shaped below about 15000 km altitude. However, according to our studies using Polar data at higher altitude, there is a lack of convergent electric field signatures at ∼20000–35000 km and consequently we suggest that the U-shaped potential contours close below this altitude range. To explain this finding, an O-shaped potential model is proposed, together with a maintenance mechanism which involves parallel energisation of middle-energy electrons by waves in the 15000–30000 km altitude range. Test particle simulations show that the presence of waves brings this “cooperative” model in quantitative agreement with both Polar and low-altitude observations. We also discuss our statistical Freja satellite studies of the observational relationship between the peak energy (voltage) and the current density in inverted-V regions. The result is that the current and voltage are sometimes correlated in the evening sector events, but almost always anticorrelated in the morning sector. This result, which is very interesting in its own right, may also have some relationship to the potential structure question.

极光电位结构和电流-电压关系:近期研究结果综述
离散的极光弧是由沉淀的加速电子引起的,有大量的观测证据表明,在大约15000千米的高度以下,相关的势结构呈u形。然而,根据我们在更高海拔使用Polar数据的研究,在~ 20000-35000公里处缺乏会聚电场特征,因此我们建议u形电位轮廓接近此高度范围。为了解释这一发现,提出了一种o形电位模型,以及一种维持机制,该机制涉及在15000-30000公里高度范围内由波平行激活中能量电子。试验粒子模拟表明,波的存在使这种“合作”模式在定量上与极地和低空观测结果一致。我们还讨论了我们的统计Freja卫星研究的峰值能量(电压)和反v区电流密度之间的观测关系。其结果是,电流和电压有时在晚上扇区事件相关,但几乎总是在早上扇区反相关。这个结果本身就很有趣,也可能与潜在的结构问题有一些关系。
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